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Motions of Chromospheric Fine Structures

Published online by Cambridge University Press:  14 August 2015

Edward N. Frazier
Edward N. Frazier*
Affiliation:
Aerospace Corporation, Los Angeles, Calif. 90009, U.S.A.

Abstract

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This review concerns itself with the measurement of the effects of chromospheric motions and the diagnosis of those motions themselves over approximately the last ten years. The different types of observational techniques are described. The different size regimes of motions are reviewed and their possible effects on observable quantities are discussed. The different types of motion in the lower chromosphere are reviewed, including microturbulence, ‘layered’ motions, and observations and interpretation of asymmetries in the core of the CaII K line. The observation of motions in Hα mottles on the disk and spicules on the limb are reviewed, from the standpoint of both line profile analysis and broad-band measurements. The interpretation of these motions and attempts to construct empirical models of chromospheric fine structures are discussed.

Type
Part IV: Motion and Excitation in the Chromosphere
Information
Symposium - International Astronomical Union , Volume 56: Chromospheric Fine Structure , 1974 , pp. 97 - 135
Copyright
Copyright © Reidel 1974 

References

Athay, R. G.: 1959, Astrophys. J. 129, 164.Google Scholar
Athay, R. G.: 1961, Astrophys. J. 134, 756.Google Scholar
Athay, R. G.: 1970a, Solar Phys. 11, 347.Google Scholar
Athay, R. G.: 1970b, Solar Phys. 12, 175.CrossRefGoogle Scholar
Athay, R. G. and Bessey, R. J.: 1964, Astrophys. J. 140, 1174.Google Scholar
Athay, R. G. and Canfield, R. C.: 1969, in Groth, and Wellman, (eds.), ‘Spectrum Formation in Stars with Steady State Extended Atmospheres’, U.S. NBS Special Report No. 332 (IAU Colloquium No. 2), p. 65.Google Scholar
Athay, R. G. and Moreton, G. E.: 1961, Astrophys. J. 131, 935.Google Scholar
Athay, R. G. and Thomas, R. N.: 1957, Astrophys. J. 125, 806.Google Scholar
Avery, L. W.: 1970, Solar Phys. 13, 301.Google Scholar
Bappu, M. K. V. and Sivaraman, K. R.: 1971, Solar Phys. 17, 316.Google Scholar
Beckers, J. M.: 1962, Australian J. Phys. 15, 327.Google Scholar
Beckers, J. M.: 1964, Thesis, Utrecht.Google Scholar
Beckers, J. M.: 1966, in Kiepenheuer, K. O. (ed.), The Fine Structure of the Solar Atmosphere , Franz Steiner Verlag, Wiesbaden.Google Scholar
Beckers, J. M.: 1968, Solar Phys. 3, 367.Google Scholar
Beckers, J. M.: 1972, Ann. Rev. Astron. Astrophys. 10, 73.CrossRefGoogle Scholar
Beebe, H. A.: 1971, Solar Phys. 17, 304.CrossRefGoogle Scholar
Beebe, H. A. and Johnson, H. R.: 1969, Solar Phys. 10, 79.CrossRefGoogle Scholar
Bhavilai, R.: 1965, Monthly Notices Royal Astron. Soc. 130, 411.Google Scholar
Bhavilai, R.: 1966, in Kiepenheuer, K. O. (ed.), The Fine Structure of the Solar Atmosphere , Franz Steiner Verlag, Wiesbaden.Google Scholar
Bray, R. J.: 1973, Solar Phys. 29, 317.Google Scholar
Canfield, R. C.: 1969, Astrophys. J. 157, 425.Google Scholar
Canfield, R. C.: 1971, Solar Phys. 20, 275.CrossRefGoogle Scholar
Cannon, C. J.: 1971, Solar Phys. 16, 314.CrossRefGoogle Scholar
Cannon, C. J.: 1971, Solar Phys. 21, 82.Google Scholar
Cannon, C. J. and Rees, D. E.: 1971, Astrophys. J. 169, 157.Google Scholar
Cram, L. E.: 1972, Solar Phys. 22, 375.CrossRefGoogle Scholar
de Jager, C.: 1959, Handbuch der Physik LII, 80.Google Scholar
Dunn, R. B.: 1960, Thesis, Harvard.Google Scholar
Dunn, R. B.: 1965, AFCRL Env. Res. Paper , No. 109.Google Scholar
Giovanelli, R. G., Michard, R., and Mouradian, Z.: 1965, Ann. Astrophys. 28, 871.Google Scholar
Grossman-Doerth, U. and von Uexküll, M.: 1971, Solar Phys. 20, 31.Google Scholar
Grossman-Doerth, U. and von Uexküll, M.: 1973, Solar Phys. 28, 319.Google Scholar
Gulyaev, R. A.: 1965, Soln. Dann. 6, 51.Google Scholar
Gulyaev, R. A. and Livshitz, M. A.: 1965, Astron. Zh. 42, 584.Google Scholar
Jones, R. A. and Rense, W. A.: 1970, Solar Phys. 15, 317.Google Scholar
Krat, V. A.: 1972, Solar Phys. 27, 39.Google Scholar
Krat, V. A. and Krat, T. V.: 1961, Izv. Pulkova 22, No. 167, 6.Google Scholar
Krat, V. A. and Krat, T. V.: 1971, Solar Phys. 17, 355.CrossRefGoogle Scholar
Kulander, J. L.: 1967, Astrophys. J. 147, 1063.Google Scholar
Kulander, J. L.: 1968, J. Quant. Spectr. Radiative Transfer 8, 273.Google Scholar
Kulander, J. L. and Jeffries, J. T.: 1966, Astrophys. J. 146, 194.Google Scholar
Leighton, R. B., Noyes, R. W., and Simon, G. W.: 1962, Astrophys. J. 135, 474.CrossRefGoogle Scholar
Linsky, J. L. and Avrett, E. H.: 1970, Publ. Astron. Soc. Pacific 82, 169.Google Scholar
Lippincott, S. L.: 1957, Smithsonian Contrib. Astrophys. 2, 15.Google Scholar
Liu, S. Y.: 1973, Preprint.Google Scholar
Liu, S. Y., Sheeley, N. R. Jr., and Smith, E. v. P.: 1972, Solar Phys. 23, 289.Google Scholar
Liu, S. Y. and Smith, E. v. P.: 1972, Solar Phys. 24, 301.Google Scholar
Livshitz, M. A.: 1966, Astron. Zh. 43, 718.Google Scholar
Loughhead, R. E.: 1973, Solar Phys. 29, 327.Google Scholar
Lynch, D. K., Beckers, J. M., and Dunn, R. B.: 1973, Solar Phys. 30, 63.Google Scholar
Mein, P.: 1971, Solar Phys. 20, 3.Google Scholar
Michard, R.: 1956, Ann. Astrophys. 19, 1.Google Scholar
Michard, R.: 1959, Ann. Astrophys. 22, 547.Google Scholar
Mouradian, Z.: 1965, Ann. Astrophys. 28, 805.Google Scholar
Mouradian, Z.: 1967, Solar Phys. 2, 258.Google Scholar
Nikolskaya, K. I.: 1967, Astron. Zh. 44, 1043.Google Scholar
Nikolsky, G. M.: 1970, Solar Phys. 12, 379.Google Scholar
Nikolsky, G. M. and Platova, A. G.: 1971, Solar Phys. 18, 403.Google Scholar
Nikolsky, G. M. and Sazanov, A. A.: 1966, Astron. Zh. 43, 928.Google Scholar
Noyes, R. W.: 1965, in Thomas, R. N. (ed.) ‘Aerodynamic Phenomena in Stellar Atmospheres’, IAU Symp. 28, 468.Google Scholar
Pasachoff, J. M.: 1970, Solar Phys. 12, 202.CrossRefGoogle Scholar
Pasachoff, J. M., Noyes, R. W., and Beckers, J. M.: 1968, Solar Phys. 5, 131.Google Scholar
Rodionov, V. V.: 1968, Vestn. Mosk. Univ. 4, 33.Google Scholar
Rush, J. H. and Roberts, W. D.: 1954, Australian J. Phys. 7, 230.Google Scholar
Skumanich, A., Smythe, C., and Frazier, E. N.: 1972, Bull. Amer. Astron. Soc. 4, 391.Google Scholar
Title, A. M.: 1966, Thesis, Calif. Inst. of Tech.Google Scholar
Vernazza, J. G., Avrett, E. H., and Loeser, R.: 1973, Astrophys. J. 184, 605.Google Scholar
Weart, S. R.: 1970, Solar Phys. 14, 310.Google Scholar
Wilson, A. M.: 1973, Preprint.Google Scholar
Wilson, P. R.: 1970, Solar Phys. 15, 139.Google Scholar
Wilson, P. R. and Evans, C. D.: 1971, Solar Phys. 18, 29.Google Scholar
Wilson, P. R., Rees, D. E., Beckers, J. M., and Brown, D. R.: 1972, Solar Phys. 25, 86.Google Scholar
Zirin, H.: 1966, The Solar Atmosphere , Blaisdell Publ. Co., Waltham.Google Scholar
Zirker, J. B.: 1962, Astrophys. J. 136, 250.Google Scholar
Zirker, J. B.: 1967, Solar Phys. 1, 204.Google Scholar